Dino Boccaletti
Theory of Orbits: Volume 1: Integrable Systems and Non-perturbative Methods - Astronomy and Astrophysics Library Dino Boccaletti Softcover reprint of hardcover 1st ed. 1996 edition

Name: Theory of Orbits: Volume 1: Integrable Systems and Non-perturbative Methods - Astronomy and Astrophysics Library
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Author: Dino Boccaletti

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Hardcover Book

1st ed. 1996. Corr. 3rd printing 2003 edition

(1996) € 90,99

Theory of Orbits: Volume 1: Integrable Systems and Non-perturbative Methods - Astronomy and Astrophysics Library

Dino Boccaletti

Softcover reprint of hardcover 1st ed. 1996 edition

Half a century ago, S. Chandrasekhar wrote these words in the preface to his l celebrated and successful book: In this monograph an attempt has been made to present the theory of stellar dy namics as a branch of classical dynamics - a discipline in the same general category as celestial mechanics. [ ... J Indeed, several of the problems of modern stellar dy namical theory are so severely classical that it is difficult to believe that they are not already discussed, for example, in Jacobi's Vorlesungen. Since then, stellar dynamics has developed in several directions and at var ious levels, basically three viewpoints remaining from which to look at the problems encountered in the interpretation of the phenomenology. Roughly speaking, we can say that a stellar system (cluster, galaxy, etc.) can be con sidered from the point of view of celestial mechanics (the N-body problem with N » 1), fluid mechanics (the system is represented by a material con tinuum), or statistical mechanics (one defines a distribution function for the positions and the states of motion of the components of the system).

405 pages, biography

Mediji	Grāmatas Paperback Book (Grāmata ar mīksto vāku un līmēto muguru)
Izlaists	2010. gada 1. decembris
ISBN13	9783642082108
Izdevēji	Springer-Verlag Berlin and Heidelberg Gm
Lapas	392
Izmēri	155 × 235 × 21 mm · 576 g
Valoda	Angļu